Numerical study of rotating relativistic stars

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The equations of structure for rotating stars in general relativity are presented and put in a form suitable for computer calculations. The results of equilibrium calculations for supermassive stars, neutron stars, and magnetically supported stars are reported, as are calculations of collapsing, rotating, and magnetized stars in the slowly changing gravitational field approximation. (auth)

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Pages: 54

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Wilson, J.R. August 25, 1975.

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Description

The equations of structure for rotating stars in general relativity are presented and put in a form suitable for computer calculations. The results of equilibrium calculations for supermassive stars, neutron stars, and magnetically supported stars are reported, as are calculations of collapsing, rotating, and magnetized stars in the slowly changing gravitational field approximation. (auth)

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Pages: 54

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  • Meeting of physics and astrophysics of neutron stars and black holes, Varenna, Italy, 14 Jul 1975

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  • Report No.: UCRL--76967
  • Report No.: CONF-750744--1
  • Grant Number: None
  • Office of Scientific & Technical Information Report Number: 4199816
  • Archival Resource Key: ark:/67531/metadc878022

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Office of Scientific & Technical Information Technical Reports

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  • August 25, 1975

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  • Sept. 21, 2016, 2:29 a.m.

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  • Oct. 18, 2016, 1:54 p.m.

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Wilson, J.R. Numerical study of rotating relativistic stars, article, August 25, 1975; Livermore, California. (digital.library.unt.edu/ark:/67531/metadc878022/: accessed January 24, 2019), University of North Texas Libraries, Digital Library, digital.library.unt.edu; crediting UNT Libraries Government Documents Department.